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Table 1.
Data sets utilized in this study.
| Data set | Description | Depth |
|---|---|---|
| MUSE-Deep | A 3D spectroscopic survey that covers 9.92 arcmin2 of the HUDF with an average exposure time of 10 h (Bacon et al. 2017). A 1 arcmin2 area near the center receives an additional 31 h of exposure time. | 3σ emission line detection limit for a point source ranges from 1.5 to 3.1 × 10−19 erg s−1 cm−1. |
| MUSE-Wide | A 3D spectroscopic survey that covers 44 1-arcmin2 fields (DR1) each with an exposure time of 1 h (Urrutia et al. 2019). | Detection limit for emission lines of a point source is 8 ×10−18 erg s−1 cm−2 Å−1. |
| GOODS Re-ionization Era wide-Area Treasury from Spitzer | Ultradeep (GREATS) imaging survey with the Spitzer Space Telescope over the GOODS-South and North (not utilized in this study) fields (Labbé et al. 2014). The exposure time over our FOV of analysis ranges from ≈70 to ≈270 h. | 5σ limiting AB magnitudes of 26.6 and 26.5 averaged over the FOV of this study in the 3.6 μm and 4.5 μm band, respectively. |
| Hubble Legacy Fields | A combination of HST imaging data taken by 31 programs over the GOODS-S field (HLF; Illingworth et al. 2016). Includes all optical ACS/WFC filters and all infrared WFC3/IR filters. The sum of the exposure time for the full data set considered is 1611 h. | 5σ limiting AB magnitudes of the nine filters (Sect. 2.3) range from 25.5 (F140W) to 28.3 (F850LP) over our FOV of analysis. |
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